Experiments on the Relative Intensities of some X-ray Lines in the L Spectrum of Tungsten and the K Spectrum of Copper

Abstract
Tungsten L series lines.—The experiments of Duane and Patterson on the strong lines in the L series of tungsten were repeated with improved apparatus, and also some of the weaker lines were studied. The value 10 obtained by Duane and Patterson for the relative intensity of Lα1 to Lα2 was confirmed. The theoretical ratio is 9. For the β group the relative intensities were found to be, β1:β2:β3:β4:β5:β6:β7:β9:β10=100 :49.3 :15.0 :7.7 :.47 :2.0 :.4 :.68 :.60 . The relative intensities of the weak lines among themselves are not very reliable on account of the faintness of the lines and the critical absorption of the target, yet it is clear that the forbidden lines β9, β10 are of the same order of intensity as β5, β7. For the γ group the relative intensities were found to be, γ1:γ2:γ3:γ4:γ5:γ6:γ8=100 :14.0 :22.3 :7.0 :3.0 :2.3 :1(?) . γ8 could not always be obtained. The determination of the intensity ratios for α1, β1 and β2, γ1 was complicated by absorption in the target. The agreement of the observed value of the intensity ratio for β3β4 with the theoretical value 2, tends to confirm Stoner's suggestion that there are twice as many electrons in the M22 orbit as in the M21. The deviation of the observed intensity ratio for γ3γ2 from 2 may be due to the influence of intervening levels.

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